Piercing of a solitonic boson star by a black hole

Detalhes bibliográficos
Autor(a) principal: Zhong, Zhen
Data de Publicação: 2023
Outros Autores: Cardoso, Vitor, Ikeda, Taishi, Zilhão, Miguel
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10773/39696
Resumo: Recently, the piercing of a mini boson star by a black hole was studied, with tidal capture and the discovery of a “gravitational atom” being reported [Cardoso et al., Phys. Rev. D 106, 044030 (2022).]. Building on this research, we extend the study by including a hexic solitonic potential and explore the piercing of a solitonic boson star by a black hole. Notably, the solitonic boson star can reach higher compactness, which one might expect could alter the dynamics in this context. Our findings suggest that even when the black hole’s size approaches the test particle limit, the solitonic boson star is easily captured by the black hole due to an extreme tidal capture process. Regardless of the black hole initial mass and velocity, our results indicate that over 85% of the boson star material is accreted. Thus, the self-interaction does not alter the qualitative behavior of the system.
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spelling Piercing of a solitonic boson star by a black holeRecently, the piercing of a mini boson star by a black hole was studied, with tidal capture and the discovery of a “gravitational atom” being reported [Cardoso et al., Phys. Rev. D 106, 044030 (2022).]. Building on this research, we extend the study by including a hexic solitonic potential and explore the piercing of a solitonic boson star by a black hole. Notably, the solitonic boson star can reach higher compactness, which one might expect could alter the dynamics in this context. Our findings suggest that even when the black hole’s size approaches the test particle limit, the solitonic boson star is easily captured by the black hole due to an extreme tidal capture process. Regardless of the black hole initial mass and velocity, our results indicate that over 85% of the boson star material is accreted. Thus, the self-interaction does not alter the qualitative behavior of the system.American Physical Society2023-11-15T15:45:21Z2023-07-05T00:00:00Z2023-07-05info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/39696eng1550-799810.1103/PhysRevD.108.084051Zhong, ZhenCardoso, VitorIkeda, TaishiZilhão, Miguelinfo:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2024-02-22T12:17:40Zoai:ria.ua.pt:10773/39696Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T03:09:51.317967Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv Piercing of a solitonic boson star by a black hole
title Piercing of a solitonic boson star by a black hole
spellingShingle Piercing of a solitonic boson star by a black hole
Zhong, Zhen
title_short Piercing of a solitonic boson star by a black hole
title_full Piercing of a solitonic boson star by a black hole
title_fullStr Piercing of a solitonic boson star by a black hole
title_full_unstemmed Piercing of a solitonic boson star by a black hole
title_sort Piercing of a solitonic boson star by a black hole
author Zhong, Zhen
author_facet Zhong, Zhen
Cardoso, Vitor
Ikeda, Taishi
Zilhão, Miguel
author_role author
author2 Cardoso, Vitor
Ikeda, Taishi
Zilhão, Miguel
author2_role author
author
author
dc.contributor.author.fl_str_mv Zhong, Zhen
Cardoso, Vitor
Ikeda, Taishi
Zilhão, Miguel
description Recently, the piercing of a mini boson star by a black hole was studied, with tidal capture and the discovery of a “gravitational atom” being reported [Cardoso et al., Phys. Rev. D 106, 044030 (2022).]. Building on this research, we extend the study by including a hexic solitonic potential and explore the piercing of a solitonic boson star by a black hole. Notably, the solitonic boson star can reach higher compactness, which one might expect could alter the dynamics in this context. Our findings suggest that even when the black hole’s size approaches the test particle limit, the solitonic boson star is easily captured by the black hole due to an extreme tidal capture process. Regardless of the black hole initial mass and velocity, our results indicate that over 85% of the boson star material is accreted. Thus, the self-interaction does not alter the qualitative behavior of the system.
publishDate 2023
dc.date.none.fl_str_mv 2023-11-15T15:45:21Z
2023-07-05T00:00:00Z
2023-07-05
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10773/39696
url http://hdl.handle.net/10773/39696
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 1550-7998
10.1103/PhysRevD.108.084051
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dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
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